ASTR112 Astrophysics: the Galaxy Prof. John Hearnshaw 2003 semester 1 Room 804, Rutherford Building...
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Transcript of ASTR112 Astrophysics: the Galaxy Prof. John Hearnshaw 2003 semester 1 Room 804, Rutherford Building...
![Page 1: ASTR112 Astrophysics: the Galaxy Prof. John Hearnshaw 2003 semester 1 Room 804, Rutherford Building Department of Physics and Astronomy email: john.hearnshaw@canterbury.ac.nz.](https://reader035.fdocuments.in/reader035/viewer/2022081603/56649f345503460f94c51a5f/html5/thumbnails/1.jpg)
ASTR112Astrophysics: the Galaxy
Prof. John Hearnshaw 2003 semester 1
Room 804, Rutherford BuildingDepartment of Physics and Astronomy
email: [email protected]
![Page 2: ASTR112 Astrophysics: the Galaxy Prof. John Hearnshaw 2003 semester 1 Room 804, Rutherford Building Department of Physics and Astronomy email: john.hearnshaw@canterbury.ac.nz.](https://reader035.fdocuments.in/reader035/viewer/2022081603/56649f345503460f94c51a5f/html5/thumbnails/2.jpg)
ASTR112 The GalaxyLecture 1
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Panorama of the Milky Way showing millions of faint stars, star clusters, gaseous nebulae and dark clouds in a great circle around the galactic equator. Galileo in 1610 first used a telescope to resolve the Milky Way into a myriad of faint stars.
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ASTR112 The GalaxyLecture 1
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The Origin of the Milky Way by Jacopo Tintorettoc. 1575
Jupiter, wishing to immortalize his infant Hercules (whose mother was the mortal Alcmene)held him to the breasts of the sleeping goddess Juno. The milk spilt and spurted upwardsto form the Milky Way
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ASTR112 The GalaxyLecture 1
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Historical introductionHistorical introductionto the Milky Way:to the Milky Way:
Some key landmarks Some key landmarks in galactic researchin galactic research
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ASTR112 The GalaxyLecture 1
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Historical introduction• William Herschel’s Galaxy of 1785
Herschel’s Galaxy cross-section was based on star counts.Fainter stars, he reasoned, indicated a greater distanceto the edge of the star system that comprised the Milky Way.
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ASTR112 The GalaxyLecture 1
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•Jacobus Kapteyn’s Galaxy, 1922 (Kapteyn’s universe)
The Sun is in the centre of Kapteyn’s universe, and thecontours show locations of equal star density
J. Kapteyn (1851-1922)
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ASTR112 The GalaxyLecture 1
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• Harlow Shapley and the distance to the centre of the Galaxy, 1918
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ASTR112 The GalaxyLecture 1
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The globular cluster47 Tucanae, one of the nearer ones to us.It contains over105 stars.
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ASTR112 The GalaxyLecture 1
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Harlow Shapley and globular clusters
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ASTR112 The GalaxyLecture 1
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• Dust clouds in the Galaxy (E.E.Barnard, M.Wolf), 1913-27
l: Barnard photo of Milky Waycentre: Dark cloud Barnard 86r: Edward Emerson Barnard (1857-1923)
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ASTR112 The GalaxyLecture 1
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• Work of Robert Trumpler on interstellar dust absorption, 1930
RobertTrumpler in1930 comparedthe distances of star clusters from angular size with those from photometry. He showed space cannot be transparentby the discrepancy found.
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ASTR112 The GalaxyLecture 1
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• Rotation of the Galaxy (Strömberg, 1924; Oort 1926)
Jan Oort (1900-92)Dutch astronomer
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ASTR112 The GalaxyLecture 1
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• Discovery of galactic spiral arms, 1951
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ASTR112 The GalaxyLecture 1
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Young open starclusters and OBassociations near the Sun show parts ofthree spiral arms, calledthe Perseus, Orionand Sagittarius arms(from outside inwards).
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ASTR112 The GalaxyLecture 1
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• Spectroscopic analysis of gaseous nebulae by William Huggins, 1864, who showed they are gas clouds of hot low density gas from their emission line spectrum
left: Orion nebularight: Sir William Huggins(1824-1910)
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ASTR112 The GalaxyLecture 1
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• Discovery of 21-cm radio radiation from cold atomic hydrogen gas clouds in disk and spiral arms of Galaxy, 1951 (21-cm radiation was predicted theoretically in 1944).
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ASTR112 The GalaxyLecture 1
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• Discovery of spiral structure from HI 21-cm map of Galaxy (Oort et al. 1958)
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ASTR112 The GalaxyLecture 1
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• Discovery of interstellar organic molecules, especially in microwave region, from 1963. The molecules include OH, CO, H2O, H2CO and C2H5OH etc.
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ASTR112 The GalaxyLecture 1
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End of lecture 1